Astrophysics and Space Science

, Volume 54, Issue 2, pp 445–452 | Cite as

The oscillation frequencies of magnetic stellar models

  • David Moss
Article
  • 27 Downloads

Abstract

A first-order perturbation theory method developed by Goossens to determine the perturbation to the eigenfrequencies of stellar models caused by the presence of a magnetic field is modified slightly, and applied to models with toroidal and poloidal fields. Some limitations of the analysis are pointed out.

Keywords

Magnetic Field Perturbation Theory Oscillation Frequency Theory Method Stellar Model 

Preview

Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

References

  1. Ferraro, V. C. A.: 1954,Astrophys. J. 119, 407.Google Scholar
  2. Gardiner, J. G.: 1951,Monthly Notices Roy. Astron. Soc. 111, 102.Google Scholar
  3. Goossens, M.: 1972,Astrophys. Space Sci. 16, 386.Google Scholar
  4. Goossens, M.: 1976a,Astrophys. Space Sci. 43, 9.Google Scholar
  5. Goossens, M.: 1976b,Astrophys. Space Sci. 44, 397.Google Scholar
  6. Goossens, M., Smeyers, P. and Denis, J.: 1976,Astrophys. Space Sci. 39, 257.Google Scholar
  7. Milsom, F. and Wright, G. A. E.: 1976,Monthly Notices Roy. Astron. Soc. 176, 307.Google Scholar
  8. Moss, D. L.: 1975,Monthly Notices Roy. Astron. Soc. 173, 141.Google Scholar
  9. Tayler, R. J. and Markey, P.: 1973,Monthly Notices Roy. Astron. Soc. 163, 77.Google Scholar
  10. Wright, G. A. E.: 1969,Monthly Notices Roy. Astron. Soc. 146, 197.Google Scholar
  11. Wright, G. A. E.: 1973,Monthly Notices Roy. Astron. Soc. 162, 339.Google Scholar

Copyright information

© D. Reidel Publishing Company 1978

Authors and Affiliations

  • David Moss
    • 1
  1. 1.Dept. of MathematicsUniversity of ManchesterEngland

Personalised recommendations